Journal
CLASSICAL AND QUANTUM GRAVITY
Volume 20, Issue 4, Pages L23-L29Publisher
IOP PUBLISHING LTD
DOI: 10.1088/0264-9381/20/4/101
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We describe a formalism for studying spherically symmetric collapse of the massless scalar field in any spacetime dimension, and for any value of the cosmological constant Lambda. The formalism is used for numerical simulations of gravitational collapse in four spacetime dimensions with negative Lambda. We observe critical behaviour at the onset of black-hole formation, and find that the critical exponent is independent of Lambda.
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